STAR Correlations and Fluctuations PWG

[Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>]

Hi Xiaofeng,

Thank you very much for your comment. The updated version is located under the same link.

Please find my comments below:

    1. Slide 3, 4, I suggest keep the same phase diagram in your talk. Now you are using two different versions.

I use 2 different phase diagrams as I need them during my talk. Fist I introduce the whole area covered by many experimental facilities , and them I move only to STAR. I would prefer to keep both.

    2. Slide 5, You may want to use a better STAR detector image, now it looks like a small toy model.

I use this plot as it shows crucial for the BES detectors. Also, because most people use the similar one, so I would like to show a different version.

    3. Slide 6, Please define the slope of the spectra.

Done

    4. Slide 8, left figure, you may mention Blast-wave model. right figure, the muB converage, you may want to only use one  : 20 ~ 720 MeV.

Done. For the right plot I have this for BES-I.

    5. Slide 23, right plot.  you may add the reference for 4.5 GeV PRC.

Done.

    6. Slide 26, please use reference PRL 126, 092301 (2021) and PRC 104.024902 (2021), PRL 128.202303 (2022). to replace the arXiv #.

Done.

Many thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 03.07.2022, o godz. 16:02:

Hi Hanna,

    Please find below the minor suggestions for your to consider.

    1. Slide 3, 4, I suggest keep the same phase diagram in your talk. Now you are using two different versions.
    2. Slide 5, You may want to use a better STAR detector image, now it looks like a small toy model.
    3. Slide 6, Please define the slope of the spectra.
    4. Slide 8, left figure, you may mention Blast-wave model. right figure, the muB converage, you may want to only use one  : 20 ~ 720 MeV.
    5. Slide 23, right plot.  you may add the reference for 4.5 GeV PRC.
    6. Slide 26, please use reference PRL 126, 092301 (2021) and PRC 104.024902 (2021), PRL 128.202303 (2022). to replace the arXiv #.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/3 18:50, Xiaofeng Luo via Star-cf-l wrote:

Hi Hanna,

    Thank you for sending this nice overview talk "Results from the BES program at STAR" to CF PWG.
    I will go through and give my comments and suggestions.
    In the meantime, since this STAR talk cover a wide topics including CME, Flow, fluctuations, HBT, di-lepton et al.,
    I would suggest you also send the overview talk to FCV and lfs-UPC group seeking for comments and suggestions.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/3 00:04, webmaster--- via Star-cf-l wrote:

Dear star-cf-l AT lists.bnl.gov members,

Hanna Zbroszczyk (hanna.zbroszczyk AT pw.edu.pl) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/60157

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--
Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867500

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